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Table C.4

Optical photometry and source extraction flag in the CFHT optical NEP catalogue of the SPICY PAH galaxies.

ID u* (mJy) g′ (mJy) r′ (mJy) i′ (mJy) z′ (mJy) Flag
F00-1 . . . 0.0541 ± 0.0001 0.1138 ± 0.0001 0.1629 ± 0.0003 0.1986 ± 0.0007 0
F01-7 . . . 0.5749 ± 0.0000 1.2348 ± 0.0000 1.6520 ± 0.0000 1.9898 ± 0.0018 2
F01-13 . . . 0.0908 ± 0.0001 0.1716 ± 0.0002 0.2359 ± 0.0004 0.2965 ± 0.0008 0
F01-15 . . . 0.1310 ± 0.0001 0.1932 ± 0.0002 0.2417 ± 0.0002 0.2729 ± 0.0008 0
F01-19 . . . 0.0119 ± 0.0001 0.0365 ± 0.0001 0.0541 ± 0.0002 0.0751 ± 0.0006 0
F02-0 0.1306 ± 0.0002 0.3128 ± 0.0003 0.4948 ± 0.0005 0.6020 ± 0.0006 0.7171 ± 0.0013 2
F02-4 0.0068 ± 0.0001 0.0221 ± 0.0001 0.0677 ± 0.0001 0.1022 ± 0.0003 0.1444 ± 0.0005 0
F02-6 0.0645 ± 0.0002 0.1796 ± 0.0002 0.3148 ± 0.0003 0.3945 ± 0.0004 0.5119 ± 0.0009 0
F02-8 0.0147 ± 0.0001 0.0412 ± 0.0001 0.1002 ± 0.0002 0.1437 ± 0.0004 0.2040 ± 0.0006 0
F02-9 0.0116 ± 0.0001 0.0260 ± 0.0001 0.0660 ± 0.0002 0.0944 ± 0.0003 0.1378 ± 0.0006 2
F02-15 0.0196 ± 0.0001 0.0478 ± 0.0001 0.1045 ± 0.0002 0.1474 ± 0.0003 0.1772 ± 0.0007 0
F02-20 0.0031 ± 0.0001 0.0049 ± 0.0001 0.0164 ± 0.0001 0.0236 ± 0.0002 0.0705 ± 0.0004 3
F02-24 0.0076 ± 0.0001 0.0270 ± 0.0001 0.0694 ± 0.0001 0.0988 ± 0.0003 0.1008 ± 0.0005 0
F03-4 . . . 0.0735 ± 0.0001 0.1164 ± 0.0001 0.1455 ± 0.0003 0.1560 ± 0.0007 2
F03-15 . . . 0.0102 ± 0.0001 0.0254 ± 0.0001 0.0395 ± 0.0002 0.0440 ± 0.0004 0
F04-0 . . . 0.5618 ± 0.0000 1.0224 ± 0.0000 1.3957 ± 0.0000 1.5981 ± 0.0015 0
F04-3 . . . 0.0697 ± 0.0001 0.1646 ± 0.0002 0.2468 ± 0.0002 0.3045 ± 0.0008 2
F04-5 . . . . . . 0.4626 ± 0.0004 0.5577 ± 0.0005 . . . 0
F04-6 . . . . . . 0.0147 ± 0.0001 0.0234 ± 0.0002 . . . 0
F04-7 . . . 0.2694 ± 0.0002 0.3908 ± 0.0004 0.5077 ± 0.0005 0.5526 ± 0.0015 0
F04-8 . . . . . . 0.0264 ± 0.0001 0.0425 ± 0.0002 . . . 0
F04-13 . . . . . . 0.1768 ± 0.0002 0.2521 ± 0.0002 . . . 0
F04-18 . . . . . . 0.0387 ± 0.0001 0.0521 ± 0.0001 . . . 0
F04-23 . . . 0.0095 ± 0.0001 0.0196 ± 0.0001 0.0256 ± 0.0002 0.0306 ± 0.0005 0
F04-24a . . . . . . . . . . . . . . . . . .
F05-10 0.0990 ± 0.0003 0.2359 ± 0.0002 0.3898 ± 0.0004 0.4699 ± 0.0004 0.5649 ± 0.0010 0
F05-23 0.0042 ± 0.0001 0.0086 ± 0.0001 0.0232 ± 0.0002 0.0396 ± 0.0003 0.0435 ± 0.0005 0
F07-11 . . . 0.0183 ± 0.0001 0.0520 ± 0.0001 0.0707 ± 0.0002 0.0898 ± 0.0005 0
F07-12 . . . 0.0309 ± 0.0001 0.0771 ± 0.0001 0.1097 ± 0.0002 0.1338 ± 0.0006 0
F08-1b . . . . . . . . . . . . . . . . . .
F08-5 . . . 0.1572 ± 0.0001 0.3045 ± 0.0003 0.4321 ± 0.0004 0.5143 ± 0.0009 2
F08-11 . . . 0.0217 ± 0.0001 0.0656 ± 0.0001 0.1070 ± 0.0003 0.1392 ± 0.0006 0
F08-14 . . . 0.0283 ± 0.0001 0.0792 ± 0.0001 0.1161 ± 0.0003 0.1444 ± 0.0008 2
F08-17 . . . 0.1020 ± 0.0001 0.1008 ± 0.0002 0.1435 ± 0.0003 0.1274 ± 0.0007 0
F08-23 . . . 0.2399 ± 0.0002 0.5181 ± 0.0005 0.7053 ± 0.0006 0.8904 ± 0.0008 0
F09-2 . . . 0.3688 ± 0.0000 0.5932 ± 0.0000 1.1663 ± 0.0000 1.0028 ± 0.0009 0
F10-8 . . . 0.0083 ± 0.0001 0.0274 ± 0.0001 0.0400 ± 0.0002 0.0583 ± 0.0006 0
F10-10 . . . 0.0075 ± 0.0001 0.0227 ± 0.0001 0.0337 ± 0.0002 0.0468 ± 0.0005 0
F10-13 . . . 0.0043 ± 0.0001 0.0101 ± 0.0001 0.0142 ± 0.0002 0.0143 ± 0.0005 3
F10-19 . . . 0.0041 ± 0.0001 0.0127 ± 0.0001 0.0218 ± 0.0002 0.0210 ± 0.0006 0
F11-7 . . . 0.0707 ± 0.0001 0.1521 ± 0.0001 0.2180 ± 0.0002 0.2635 ± 0.0007 0
F11-11 . . . 0.0633 ± 0.0001 0.1073 ± 0.0001 0.1426 ± 0.0003 0.1586 ± 0.0006 0
F11-19 . . . 0.1337 ± 0.0001 0.3020 ± 0.0003 0.4274 ± 0.0004 0.5521 ± 0.0010 0
F11-23 . . . 0.0682 ± 0.0001 0.1460 ± 0.0001 0.2055 ± 0.0002 0.2604 ± 0.0007 0
F20-3 . . . 0.1723 ± 0.0002 0.3287 ± 0.0003 0.4639 ± 0.0004 0.5749 ± 0.0011 0
F20-10 . . . 0.0130 ± 0.0001 0.0347 ± 0.0001 0.0492 ± 0.0002 0.0760 ± 0.0006 0
F21-1 . . . 0.1057 ± 0.0001 0.2423 ± 0.0002 0.3330 ± 0.0003 0.4305 ± 0.0004 0
F21-20 . . . 0.0049 ± 0.0001 0.0168 ± 0.0001 0.0272 ± 0.0002 0.0354 ± 0.0006 0

Notes. The flags are 0 for clear detection, 1 for having neighbours, 2 for being blended, and 3 for both 1 and 2 (see Hwang et al. 2007 for more).

(a)

This source is damaged due to a nearby bright and saturated star on the CFHT image, and is not catalogued.

(b)

This source falls on one of CCD gaps on the CFHT image, and is not catalogued.

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